Table 5
Summary of model parameters. For details on the parameter definitions see Robitaille et al. (2006).
| 3003929 | 3005903 | 3008813 | 3012934 | |||||||
|
|
||||||||||
| Inclination | 76 | 81 | 63 | 70 | 76 | 81 | 57 | 63 | 70 | 76 |
| Angle [°] | ||||||||||
| SED fitting | 141 | 189 | 190 | 153 | 123 | 151 | 194 | 199 | 189 | 188 |
| χ 2 | ||||||||||
| distance | 1905 | 1995 | 2291 | 2291 | 2291 | 2188 | 2188 | 2188 | 2089 | 1995 |
| [ pc ] | ||||||||||
| A ν | 134 | 587 | 19 | 18 | 17 | 94 | 19 | 18 | 19 | 27 |
| (total) | ||||||||||
| A ν | 13 | 12 | 19 | 18 | 17 | 12 | 19 | 18 | 19 | 16 |
| (interstellar) | ||||||||||
| stellar | 4.9 | 5.1 | 5.1 | 5.1 | 5.1 | 5.1 | 4.8 | 4.8 | 4.8 | 4.8 |
| radius [R ⊙ ] | ||||||||||
| stellar | 15 | 16 | 16 | 16 | 16 | 16 | 14 | 14 | 14 | 14 |
| mass [M⊙] | ||||||||||
| stellar | 31 000 | 32000 | 32 000 | 32 000 | 32000 | 32 000 | 31 000 | 31000 | 31 000 | 31 000 |
| temperature [K] | ||||||||||
| Luminosity | 20 700 | 25 900 | 25 000 | 25 000 | 25 000 | 25 000 | 17 700 | 17 700 | 17 700 | 17 700 |
| (total, [L ⊙ ]) | ||||||||||
| envelope accr. | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 | 0 |
| rate [M⊙/yr] | ||||||||||
| disk mass | 9 × 10-2 | 4 × 10-2 | 2 × 10-2 | 2 × 10-2 | 2 × 10-2 | 2 × 10-2 | 6 × 10-2 | 6 × 10-2 | 6 × 10-2 | 6 × 10-2 |
| [ M⊙ ] | ||||||||||
| disk inner | 2 | 6 | 8 | 8 | 8 | 8 | 5 | 5 | 5 | 5 |
| radius [Rsub] | ||||||||||
| disk inner | 26 | 84 | 99 | 99 | 99 | 99 | 55 | 55 | 55 | 55 |
| radius [AU] | ||||||||||
| disk accr. | 8 × 10-08 | 3 × 10-6 | 2 × 10-7 | 2 × 10-7 | 2 × 10-7 | 2 × 10-7 | 5 × 10-7 | 5 × 10-7 | 5 × 10-7 | 5 × 10-7 |
| rate [M⊙/yr] | ||||||||||
| disk flaring | 1.15 | 1.04 | 1.10 | 1.10 | 1.10 | 1.10 | 1.10 | 1.10 | 1.10 | 1.10 |
| parameter β | ||||||||||
Notes. Note that the total extinction given in the table is the sum of
the interstellar and intrinsic extinction. The intrinsic extinction for disk-like
structures is given for the direct line of sight; hence, it depends considerably on
the inclination and flaring of the disk. If the total and interstellar extinction
are equal on the other hand, this indicates a direct line of sight to the central
stellar source. Robitaille et al. (2006)
state that the disk structure is given by: 
where
h ∝ ϖβ and
α = β + 1.
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